Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientist
Physics
High Energy Physics
High Energy Physics - Phenomenology
Scientist
Ohio State
ITP, Beijing
Beijing, Inst. Theor. Phys.
National Astronomical Observatories, CAS;
Beijing Astronomical Observatory
National Astronomical Observatories, China
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China
Department of Land Surveying and Geo-Informatics, The Hong Kong Polytechnic University, Hong Kong, SAR, China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China
National Astronomical Observatoires, Chinese Academy of Sciences, 20A, Datun Road, Chaoyang, 100012 Beijing, People's Republic of China Astronomical Observatory, Chinese Academy of Sciences, Datun Road 20A, Chaoyang, Beijing 100012, P. R. Chin; National Astronomical Observatoires, Chinese Academy of Sciences, Datun Road 20A, Chaoyang, Beijing 100012, P. R. China; Department of Astronomy, Beijing Normal University, Beijing 100875, P. R. China
National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, China Astronomical Observatory, Chinese Academy of Sciences, Datun Road 20A, Chaoyang, Beijing 100012, P.R. Chin; National Astronomical Observatoires, Chinese Academy of Sciences, Datun Road 20A, Chaoyang, Beijing 100012, P.R. China; Department of Astronomy, Beijing Normal University, Beijing 100875, P.R. China.
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, PR China; National Astronomical Observatoires, Chinese Academy of Sciences, Beijing 100012, PR China
National Astronomical Observatoires, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100012, China
A Comparative Study on Lithium Abundances in Solar--Type Stars With and Without Planets
A Comprehensive Four-Quark Interpretation of D_s(2317), D_s(2457) and D_s(2632)
A hybrid method to determine a local geoid model -- Case study
A Substellar Companion to the Intermediate-Mass Giant 11 Com
Abundance Pattern of Metal-Rich Stars from 14 Old and 24 Young Stars
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